XMM-Newton – NuSTAR monitoring campaign of the Seyfert 1 galaxy IC 4329A

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Fig. 8.

Unfolded data plus best-fitting model (upper panels) and ratio residuals (lower panels) for the X-ray broadband observations of IC 4329A when the best-fitting model (Model A) is applied. We show all the model components as in Fig. 7 (see Sect. 4 for more details).

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